Heat Transfer Mechanisms — Question 8

Section 18-11 · Physics pages 3026–3027

Question 8 Convection and radiation act together at a heated surface Use σ = 5.67 × 10−8 W/(m2K4). A uniform surface with area .100 m2 receives steady heating power 180 W. It loses energy by convection to air at 300 K with h = 10.0 W/(m2K) and by radiation to a large black enclosure at 300 K with emissivity .800. Neglect all other transfers. surface 180 W convection radiation Schematic; labels, not drawing lengths, specify the data. (a) Write the equilibrium equation and solve numerically for surface temperature. (b) At the equilibrium, find each loss contribution. Determine the local change in equilibrium temperature per extra watt of heating by differentiating the balance.
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Question 8 - Solution Convection and radiation act together at a heated surface surface 180 W convection radiation (a) Method and calculation f(T) = hA(T −300) + ϵσA(T 4 −3004) −180 = 0. f(T) = (T −300) + 4.536 × 10−9(T 4 −3004) −180. f(400) = −.620 W, f′(T) = 1 + 1.8144 × 10−8T 3. Newton iteration Tn+1 = Tn −f(Tn)/f′(Tn) gives T ≈400.28671 K. (b) Interpretation and further calculation Pconv = T −300 ≈100.28671 W, Prad = 180 −Pconv ≈79.71329 W. dT dP = 1 hA + 4ϵσAT 3 ≈.46217 K/W. The derivative is positive, so the equilibrium is unique above 300 K and a temperature increase strengthens the restoring heat loss. Physical check Loss mechanisms add as powers at the same surface temperature; their coefficients should not be averaged.

Question 8

Convection and radiation act together at a heated surface

Use σ=5.67×10−8W/(m2K4)\sigma=5.67\times10^{-8}\,\mathrm{W/(m^2K^4)}. A uniform surface with area .100m2.100\,\mathrm{m^2} receives steady heating power 180 W. It loses energy by convection to air at 300 K with h=10.0W/(m2K)h=10.0\,\mathrm{W/(m^2K)} and by radiation to a large black enclosure at 300 K with emissivity .800. Neglect all other transfers.

Diagram shown in the original SVG worksheet.

  1. Write the equilibrium equation and solve numerically for surface temperature.

  2. At the equilibrium, find each loss contribution. Determine the local change in equilibrium temperature per extra watt of heating by differentiating the balance.

Question 8 - Solution

Convection and radiation act together at a heated surface

Diagram shown in the original SVG worksheet.

(a) Method and calculation

f(T)=hA(T−300)+ϵσA(T4−3004)−180=0.f(T)=hA(T-300)+\epsilon\sigma A(T^4-300^4)-180=0.f(T)=(T−300)+4.536×10−9(T4−3004)−180.f(T)=(T-300)+4.536\times10^{-9}(T^4-300^4)-180.f(400)=−.620W,f′(T)=1+1.8144×10−8T3.f(400)=-.620\,\mathrm W,\quad f\prime(T)=1+1.8144\times10^{-8}T^3.Newton iteration Tn+1=Tn−f(Tn)/f′(Tn)T_{n+1}=T_n-f(T_n)/f\prime(T_n) gives T≈400.28671T\approx400.28671 K.

(b) Interpretation and further calculation

Pconv=T−300≈100.28671W,Prad=180−Pconv≈79.71329W.P_{\mathrm{conv}}=T-300\approx100.28671\,\mathrm W,\quad P_{\mathrm{rad}}=180-P_{\mathrm{conv}}\approx79.71329\,\mathrm W.dTdP=1hA+4ϵσAT3≈.46217K/W.\frac{dT}{dP}=\frac1{hA+4\epsilon\sigma AT^3}\approx.46217\,\mathrm{K/W}.The derivative is positive, so the equilibrium is unique above 300 K and a temperature increase strengthens the restoring heat loss.

Physical check

Loss mechanisms add as powers at the same surface temperature; their coefficients should not be averaged.